Acceleration of cosmic rays and gamma-ray emission from supernova remnant/molecular cloud associations
arXiv:1504.05719 · doi:10.1051/epjconf/201510502001
Abstract
The gamma-ray observations of molecular clouds associated with supernova remnants are considered one of the most promising ways to search for a solution of the problem of cosmic ray origin. Here we briefly review the status of the field, with particular emphasis on the theoretical and phenomenological aspects of the problem.
Invited talk at SUGAR2015